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Record W4306896922 · doi:10.1051/0004-6361/202244791

TOI-3884 b: A rare 6-<i>R</i><sub>E</sub>planet that transits a low-mass star with a giant and likely polar spot

2022· article· en· W4306896922 on OpenAlexfundno aff
J. M. Almenara, X. Bonfıls, T. Forveille, N. Astudillo-Defru, David R. Ciardi, Richard P. Schwarz, Karen A. Collins, Marion Cointepas, Michael B. Lund, F. Bouchy, D. Charbonneau, R. F. Díaz, X. Delfosse, R. C. Kidwell, M. Kunimoto, David W. Latham, J. J. Lissauer, F. Murgas, G. Ricker, Sara Seager, M. Vezie, David Watanabe

Bibliographic record

VenueAstronomy and Astrophysics · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersPlanetary Science DivisionAgencia Estatal de InvestigaciónScience Mission DirectorateSmithsonian Astrophysical ObservatoryUniversity of EdinburghMax-Planck-Institut für AstronomieAmes Research CenterCentre National de la Recherche ScientifiqueSpace Telescope Science InstituteEuropean Southern ObservatoryMinistry of Science, ICT and Future PlanningQueen's UniversityAgence Nationale de la RechercheLos Alamos National LaboratoryEuropean Space AgencyJohns Hopkins UniversityGordon and Betty Moore FoundationQueen's University BelfastNational Science FoundationNational Aeronautics and Space AdministrationEötvös Loránd TudományegyetemCalifornia Institute of TechnologyNational Central UniversityDurham UniversitySmithsonian Institution
KeywordsPhysicsExoplanetPlanetAstronomyAstrophysicsPhotometry (optics)ObservatoryTransit (satellite)Stars

Abstract

fetched live from OpenAlex

The Transiting Exoplanet Survey Satellite mission identified a deep and asymmetric transit-like signal with a periodicity of 4.5 days orbiting the M4 dwarf star TOI-3884. The signal has been confirmed by follow-up observations collected by the ExTrA facility and Las Cumbres Observatory Global Telescope, which reveal that the transit is chromatic. The light curves are well modelled by a host star having a large polar spot transited by a 6-REplanet. We validate the planet with seeing-limited photometry, high-resolution imaging, and radial velocities. TOI-3884 b, with a radius of 6.00 ± 0.18 RE, is the first sub-Saturn planet transiting a mid-M dwarf. Owing to the host star’s brightness and small size, it has one of the largest transmission spectroscopy metrics for this planet size and becomes a top target for atmospheric characterisation with theJames WebbSpace Telescope and ground-based telescopes.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.004
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0000.000
Open science0.0000.001
Research integrity0.0010.000
Insufficient payload (model declined to judge)0.0020.001

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.005
GPT teacher head0.164
Teacher spread0.159 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations31
Published2022
Admission routes1
Has abstractyes

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